期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 300, 期 1-3, 页码 107-117出版社
SPRINGER
DOI: 10.1007/s10509-005-1197-4
关键词
accretion; accretion disks; black hole physics; X-rays; stars; X-rays; binaries
We discuss the evolution of black hole transients on the basis of a few systems that were intensively observed with the Rossi X-ray Timing Explorer (rxte). We focus on the global evolution and the observed state transitions. Rather than giving a numerical recipe for classifying observations, we try to identify times during outbursts at which clear changes occur in the X-ray variability, X-ray spectral, or multi-wavelength properties.
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